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Starting from a locked thread I tried to work the gravity of a body of mass ##M## on another body starting from infinity to some distance ##d## from the gravitating body.
We have from the SR 2nd Newton law that:
\gamma^3 a = \frac{GM}{r^2}
writting a= \frac{dv}{dt}= v \frac{dv}{dr} = \frac{1}{2} \frac{dv^2}{dr}
Naming v^2/c^2= x the above relation becomes:
\frac{dx}{(1-x)^{3/2}}= \frac{2GM}{c^2 r^2}dr
Integrating:
\int_{0}^{x_d}\frac{dx}{(1-x)^{3/2}}= \int_{\infty}^{d} \frac{2GM}{c^2 r^2}dr
\frac{2}{\sqrt{1-x_d}}-2= - \frac{2GM}{c^2 d}
x_d=1- \Big( 1- \frac{GM}{c^2 d}\Big)^{-2}
And so:
v(d)= c \bigg[ 1- \Big( 1- \frac{GM}{c^2 d}\Big)^{-2} \bigg]^{1/2}
I tried plotting this solution as v(d), the good part is that v<c for all distances however I don't understand why for d=GM/c^2 I'm obtaining an infinity (and worse- in the imaginary regime)? By the way, that's the Schwarzschild radius...
Even worse, if I set \frac{GM}{c^2}=1 the plot of \beta = v/c = \bigg[ 1- \Big( 1- \frac{1}{d}\Big)^{-2} \bigg]^{1/2} is given in my attachment...and doesn't seem to have a real solution away from 1?
We have from the SR 2nd Newton law that:
\gamma^3 a = \frac{GM}{r^2}
writting a= \frac{dv}{dt}= v \frac{dv}{dr} = \frac{1}{2} \frac{dv^2}{dr}
Naming v^2/c^2= x the above relation becomes:
\frac{dx}{(1-x)^{3/2}}= \frac{2GM}{c^2 r^2}dr
Integrating:
\int_{0}^{x_d}\frac{dx}{(1-x)^{3/2}}= \int_{\infty}^{d} \frac{2GM}{c^2 r^2}dr
\frac{2}{\sqrt{1-x_d}}-2= - \frac{2GM}{c^2 d}
x_d=1- \Big( 1- \frac{GM}{c^2 d}\Big)^{-2}
And so:
v(d)= c \bigg[ 1- \Big( 1- \frac{GM}{c^2 d}\Big)^{-2} \bigg]^{1/2}
I tried plotting this solution as v(d), the good part is that v<c for all distances however I don't understand why for d=GM/c^2 I'm obtaining an infinity (and worse- in the imaginary regime)? By the way, that's the Schwarzschild radius...
Even worse, if I set \frac{GM}{c^2}=1 the plot of \beta = v/c = \bigg[ 1- \Big( 1- \frac{1}{d}\Big)^{-2} \bigg]^{1/2} is given in my attachment...and doesn't seem to have a real solution away from 1?
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